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Interacting supernovae and supernova impostors. LSQ13zm: An outburst heralds the death of a massive star
Tartaglia L., Pastorello A., Sullivan M., Baltay C., Rabinowitz D., Nugent P., Drake A., Djorgovski S., Gal-Yam A., Fabrika S., Barsukova E., Goranskij V., Valeev A., Fatkhullin T., Schulze S., Mehner A., Bauer F., Taubenberger S., Nordin J., Valenti S., Howell D., Benetti S., Cappellaro E., Fasano G., Elias-Rosa N., Barbieri M., Bettoni D., Harutyunyan A., Kangas T., Kankare E., Martin J., Mattila S., Morales-Garoffolo A., Ochner P., Rebbapragada U., Terreran G., Tomasella L., Turatto M., Verroi E., Woźniak P.
') followed by a much brighter outburst ('2013b') three weeks later, that we argue to be the genuine supernova
Non-thermal radio supernova remnants of exiled Wolf-Rayet stars
Meyer D.M.A., Pohl M., Petrov M., Oskinova L.
eventually die with a supernova explosion. The morphology of the resulting remnant is largely governed
SN2015bh in NGC 2770: LBV core collapse in merging of binary system components
Goranskij V., Barsukova E., Valeev A., Tsvetkov D., Volkov I., Metlov V., Zharova A.
into the supernova phase and got the name SN2015bh. Medium-resolution spectral observations were carried out between
Type Ia supernovae 2014J and 2011fe at the nebular phase
Bikmaev I., Chugai N., Sunyaev R., Churazov E., Khamitov I., Sakhibullin N., Galeev A., Akhmetkhanova A.
of the nebular spectra for two nearby type Ia supernovae (SN 2014J and SN 2011fe). For the overall picture, we
Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
Kubankin, A., Nikulin, I., Oleinik, A., Shchagin, A.
, will be sensitive also to core-collapse supernova neutrinos, via coherent elastic neutrino-nucleus scattering
Type Ia supernovae 2014J and 2011fe at the nebular phase
Bikmaev I., Chugai N., Sunyaev R., Churazov E., Khamitov I., Sakhibullin N., Galeev A., Akhmetkhanova A.
of the nebular spectra for two nearby type Ia supernovae (SN 2014J and SN 2011fe). For the overall picture, we
Interacting supernovae and supernova impostors. LSQ13zm: An outburst heralds the death of a massive star
Tartaglia L., Pastorello A., Sullivan M., Baltay C., Rabinowitz D., Nugent P., Drake A., Djorgovski S., Gal-Yam A., Fabrika S., Barsukova E., Goranskij V., Valeev A., Fatkhullin T., Schulze S., Mehner A., Bauer F., Taubenberger S., Nordin J., Valenti S., Howell D., Benetti S., Cappellaro E., Fasano G., Elias-Rosa N., Barbieri M., Bettoni D., Harutyunyan A., Kangas T., Kankare E., Martin J., Mattila S., Morales-Garoffolo A., Ochner P., Rebbapragada U., Terreran G., Tomasella L., Turatto M., Verroi E., Woźniak P.
') followed by a much brighter outburst ('2013b') three weeks later, that we argue to be the genuine supernova
LCDM-model and Universe filled with radiation. Comparison with the data from the SAI Supernovae Catalog
Gavrikov A.S., Saha B.
filled with radiation, based on data from the SAI Supernovae Catalog. Thus, the task is to select a set
SN2015bh in NGC 2770: LBV core collapse in merging of binary system components
Goranskij V., Barsukova E., Valeev A., Tsvetkov D., Volkov I., Metlov V., Zharova A.
into the supernova phase and got the name SN2015bh. Medium-resolution spectral observations were carried out between
GAMMA RAYS from TYPE Ia SUPERNOVA SN 2014J
Churazov E., Sunyaev R., Isern J., Bikmaev I., Bravo E., Chugai N., Grebenev S., Jean P., Knödlseder J., Lebrun F., Kuulkers E.
observations of Type Ia supernova SN 2014J, covering the period 19-162 days after the explosion, has been

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